Parallax Estimates Using Electronic Techniques

Details Parallax Estimates Using Electronic Techniques Parallax Estimates Using Electronic Techniques

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983nssl.conf...75g&link_type=abstract

The Nearby Stars and the Stellar Luminosity Function, Proceedings of IAU Colloquium No. 76 held 13-16 June 1983 at Wesleyan Univ

Computer Science

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3

Scientific paper

The high precision of electronic detectors reveal parallactic motion more quickly and potentially more accurately than previously possible. Stars with distances of up to 500 pc have a greater total parallactic motion that the error of a single observation made with the Multichannel Astrometric Photometer (MAP). This paper presents several plots of the MAP's observational performance as functions of atmospheric conditions, sky brightness, Ronchi ruling frequency and clear to dark line ratio.

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